{"title":"太阳周期变化的内带质子带结构","authors":"A. Vampola, M. Lauriente","doi":"10.1109/CHERBS.1997.660258","DOIUrl":null,"url":null,"abstract":"Using a 2-D (longitude and latitude) cross-correlation between sets of SEUs from the TOMS satellite in the inner zone in 1992 and 1995, it is shown that the centroid of the energetic proton ensemble causing these SEUs moved to lower L (1.26 vs. 1.29 for the protons) during this period. This change in the energetic proton distribution at low altitude is due to the change in atmospheric scale height during the declining phase of the solar cycle. The AP8 model does not predict this change in the location in L of the peak in the inner zone protons.","PeriodicalId":197895,"journal":{"name":"Conference on the High Energy Radiation Background in Space. Workshop Record","volume":"1 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1997-07-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"4","resultStr":"{\"title\":\"Solar cycle variations in the inner zone proton belt configuration\",\"authors\":\"A. Vampola, M. Lauriente\",\"doi\":\"10.1109/CHERBS.1997.660258\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Using a 2-D (longitude and latitude) cross-correlation between sets of SEUs from the TOMS satellite in the inner zone in 1992 and 1995, it is shown that the centroid of the energetic proton ensemble causing these SEUs moved to lower L (1.26 vs. 1.29 for the protons) during this period. This change in the energetic proton distribution at low altitude is due to the change in atmospheric scale height during the declining phase of the solar cycle. The AP8 model does not predict this change in the location in L of the peak in the inner zone protons.\",\"PeriodicalId\":197895,\"journal\":{\"name\":\"Conference on the High Energy Radiation Background in Space. Workshop Record\",\"volume\":\"1 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1997-07-22\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"4\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Conference on the High Energy Radiation Background in Space. Workshop Record\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/CHERBS.1997.660258\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Conference on the High Energy Radiation Background in Space. Workshop Record","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/CHERBS.1997.660258","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 4
摘要
利用1992年和1995年TOMS卫星内区seu组的二维(经纬度)互相关分析表明，在此期间，导致这些seu的高能质子系综质心向低L移动(1.26 vs. 1.29)。低空高能质子分布的这种变化是由于太阳活动周期下降阶段大气尺度高度的变化。AP8模型没有预测到内区质子峰在L中的位置变化。
Solar cycle variations in the inner zone proton belt configuration
Using a 2-D (longitude and latitude) cross-correlation between sets of SEUs from the TOMS satellite in the inner zone in 1992 and 1995, it is shown that the centroid of the energetic proton ensemble causing these SEUs moved to lower L (1.26 vs. 1.29 for the protons) during this period. This change in the energetic proton distribution at low altitude is due to the change in atmospheric scale height during the declining phase of the solar cycle. The AP8 model does not predict this change in the location in L of the peak in the inner zone protons.
求助内容：
应助结果提醒方式：
京公网安备 11010802042870号
